Difference between revisions of "Black Hole"

From Discovery Wiki
Jump to navigationJump to search
m
m
Line 3: Line 3:
 
A black hole is a theoretical entity predicted by the equations of general relativity. A black hole is formed when a star of sufficient mass undergoes gravitational collapse, with most or all of its mass compressed into a sufficiently small area of space, causing infinite spacetime curvature at that point (a ''singularity''). Such a massive spacetime curvature allows nothing, not even light, to escape from the ''event horizon'' or border.
 
A black hole is a theoretical entity predicted by the equations of general relativity. A black hole is formed when a star of sufficient mass undergoes gravitational collapse, with most or all of its mass compressed into a sufficiently small area of space, causing infinite spacetime curvature at that point (a ''singularity''). Such a massive spacetime curvature allows nothing, not even light, to escape from the ''event horizon'' or border.
  
Only one black hole is present in Sirius, located in [[Omicron-85]]. If the star has a low mass for a black hole, they can become [[Neutron Star|Neutron Stars]]. Several theories have been made on the stars of [[Omega-11]] and [[New Berlin]], if they would become black holes or neutron stars, or if they will just collapse forming a black object.
+
Only one black hole is present in Sirius, [[Razgriz Black Hole|located]] in [[Omicron-85]]. If the star has a low mass for a black hole, they can become [[Neutron Star|Neutron Stars]]. Several theories have been made on the stars of [[Omega-11]] and [[New Berlin]], if they would become black holes or neutron stars, or if they will just collapse forming a black object.
  
 
Getting close to the ''event horizon'' will result in nearly instant death.
 
Getting close to the ''event horizon'' will result in nearly instant death.

Revision as of 18:35, 1 February 2016

WARNING, NAVIGATIONAL HAZARD!

A black hole is a theoretical entity predicted by the equations of general relativity. A black hole is formed when a star of sufficient mass undergoes gravitational collapse, with most or all of its mass compressed into a sufficiently small area of space, causing infinite spacetime curvature at that point (a singularity). Such a massive spacetime curvature allows nothing, not even light, to escape from the event horizon or border.

Only one black hole is present in Sirius, located in Omicron-85. If the star has a low mass for a black hole, they can become Neutron Stars. Several theories have been made on the stars of Omega-11 and New Berlin, if they would become black holes or neutron stars, or if they will just collapse forming a black object.

Getting close to the event horizon will result in nearly instant death.

See Also


Razgriz Black Hole

Neutron Star